Correction: Corrigendum: Slowly fading super-luminous supernovae that are not pair-instability explosions

Autor: Christopher W. Stubbs, Jesper Sollerman, M. McCrum, S. Valenti, Dan Milisavljevic, K. C. Chambers, E. A. Magnier, A. Morales-Garoffolo, Matt Nicholl, Nick Kaiser, Francesco Taddia, P. A. Price, S. J. Smartt, Giorgos Leloudas, S. Benetti, Seppo Mattila, Ting-Wan Chen, Morgan Fraser, David Young, R. P. Kudritzki, W. S. Burgett, Gautham Narayan, Alicia Soderberg, Enrico Cappellaro, Christopher M. Waters, R. Lunnan, L. Tomasella, Suvi Gezari, K. W. Smith, Yuji Urata, Anders Jerkstrand, S. Rodney, Edo Berger, Erkki Kankare, M. T. Botticella, Nigel Metcalfe, Ryan J. Foley, W. M. Wood-Vasey, John L. Tonry, M. E. Huber, David W. Wright, H. Flewelling, R. Chornock, C. Inserra, Daniel Scolnic, Nancy Elias-Rosa, Armin Rest, D. A. Howell, Rubina Kotak, Adam G. Riess, W. E. Sweeney, S. Taubenberger, Stuart A. Sim, A. Pastorello, R. P. Kirshner, F. Bresolin, T. Kangas, John Morgan, Nathan Edward Sanders, R. Margutti
Rok vydání: 2016
Předmět:
Zdroj: Nature. 539:598-598
ISSN: 1476-4687
0028-0836
Popis: Nature 502, 346–349 (2013); doi:10.1038/nature12569 In this Letter, we have identified an important error affecting Fig. 4 and Extended Data Fig. 6, as well as the values of some parameters derived from our model fits. We stress that this error in no way affects the discussion or the conclusions. Inbuilding the bolometric light curve of the superluminous supernova PTF 12dam, our code assumed that photometry from the Swift satellite was calibrated in the Vega magnitude system.
Databáze: OpenAIRE
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